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1. The Interior Structure of the Sun
2. First hint: solar granulation as evidence of convection
3. The scale of solar granulation
4. Movie of solar granulation
5. Our knowledge of the solar interior
6. Stellar interior slides from textbook (17.1)
7. How can we know the structure of the Sun below the photosphere? Application of the laws of physics (equations of stellar structure), find solution consistent with mass and radius of Sun
Measure “eigenmodes” of the Sun (see how fast it jiggles
Results for how the sun is put together
8. Physical properties 1: density Units: mass/volume
Grams/cc
water…1 grams/cc
rock… about 3 grams/cc
Lead…11.3 grams/cc
9. Physical properties 2: temperature Units: degrees centrigrade
Temperature Kelvin: degrees C about absolute zero
Temperature of this room: 295K
Boiling point of water: 373 K
Surface temperature of Sun 5800K
10. Distribution of density inside the Sun
11. Distribution of temperature inside the Sun
12. The interior of the Sun is a region of extreme physical conditions
13. Next topic: what is the luminosity of the Sun telling us? Luminosity = 3.847X1026 Watts
What fuel cycle could provide this?
What fuel cycle could provide this for the lifetime of the Sun?